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Occultation of X-rays from Scorpius X-1 by small trans-neptunian objects

Hsiang-Kuang Chang (), Sun-Kun King, Jau-Shian Liang, Ping-Shien Wu, Lupin Chun-Che Lin and Jeng-Lun Chiu
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Hsiang-Kuang Chang: National Tsing Hua University
Sun-Kun King: Institute of Astronomy and Astrophysics, Academia Sinica
Jau-Shian Liang: National Tsing Hua University
Ping-Shien Wu: Institute of Astronomy, National Tsing Hua University
Lupin Chun-Che Lin: National Tsing Hua University
Jeng-Lun Chiu: National Tsing Hua University

Nature, 2006, vol. 442, issue 7103, 660-663

Abstract: Solar System minnows Scorpius X-1 (Sco X1) has an important place in the history of astronomy as, apart from the Sun, it was the first cosmic X-ray source ever detected. It now has a new claim to fame: small but significant dips in its X-ray light curves obtained by the Rossi X-ray Timing Explorer satellite may represent the first ever observation of small (less than 100 metre diameter) trans-neptunian objects (TNOs). The irregularities occur at millisecond time scales and are almost certainly caused by occultation of tiny TNOs. Since the first discovery of a Kuiper belt object in 1992, nearly a thousand more TNOs have been found. The ones that have been seen are hundreds to several thousand kilometres in diameter but many smaller objects have been expected to exist.

Date: 2006
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DOI: 10.1038/nature04941

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